Massless “just-so” solution to the solar neutrino problem
- 8 October 2001
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 64 (9) , 097301
- https://doi.org/10.1103/physrevd.64.097301
Abstract
We study the effect of the nonresonant, vacuum oscillationlike neutrino flavor conversion induced by nonstandard flavor changing and nonuniversal flavor diagonal neutrino interactions with electrons in the Sun. We have found an acceptable fit for the combined analysis for the solar experiments total rates, the Super-Kamiokande energy spectrum and zenith angle dependence. Phenomenological constraints on nonstandard flavor changing and nonuniversal flavor diagonal neutrino interactions are considered.Keywords
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This publication has 29 references indexed in Scilit:
- First results from GNONuclear Physics B - Proceedings Supplements, 2001
- Solar neutrino results from SAGENuclear Physics B - Proceedings Supplements, 2001
- Solar neutrino results from Super-KamiokandeNuclear Physics B - Proceedings Supplements, 2001
- GNO solar neutrino observations: results for GNO IPhysics Letters B, 2000
- How uncertain are solar neutrino predictions?Physics Letters B, 1998
- Measurement of the Solar Electron Neutrino Flux with the Homestake Chlorine DetectorThe Astrophysical Journal, 1998
- Mikheyev-Smirnov-Wolfenstein effect with flavor-changing neutrino interactionsPhysical Review D, 1991
- On the MSW effect with massless neutrinos and no mixing in the vacuumPhysics Letters B, 1991
- Neutrino oscillations and stellar collapsePhysical Review D, 1979
- Neutrino oscillations in matterPhysical Review D, 1978